Do we understand IBM parameters?

“…However, the special choice of effective nucleon inter actions seems to lead to implicit consideration of non collective phonons. These were explicitly considered within IBM2 in [9].…”

Section: Introductionmentioning

confidence: 99%

Microscopic description of absolute values for B(E2) within IBM

Efimov

Mikhajlov

2013

Bull. Russ. Acad. Sci. Phys.

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“…As the image of d-bosons we employ the quadrupole phonons of MQRPA with the lowest energy. As shown by IBM2 [16] and our [12] calculations, in order to obtain the realistic values of IBM parameters one has to renormalize them, taking into account the connection of the collective D-phonon or d-boson space with phonons of higher energies and angular momenta L≥2. So all calculations here for Xe isotopes and in Ref.…”

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confidence: 99%

Collective states of even Xe isotopes in IBM+MQRPA

Efimov

Mikhajlov

2016

EPJ Web of Conferences

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Abstract. A modification of the Quasiparticle Random Phase Approximation (QRPA) with small ground state correlations is suggested. The lowest energy phonon is used as the image of d-boson of the Interacting Boson Model 1 (IBM1) and applied to microscopical calculations of the IBM1 parameters. Results are compared with experimental data for Xe isotopes.The Quasiparticle Random Phase Approximation (QRPA) is one of the widely used methods for description of semimagic and deformed nuclei [1]. Application of this approximation is quite correct in those cases when the Ground State Correlations (GSC) i.e. the distinction between the quasiparticle vacuum (QV) and the RPA-phonon vacuum (PV), exist but are rather small. Quantitatively it means, e.g., that Σψ 2 Σϕ 2 , ψ, ϕ being amplitudes of the RPA D μ -phonons (μ=0, ±1, ±2)Futher, we'll work with the QRPA-phonons composed of the Bogoliubov quasiparticles. In Eq.(1), a + i , a k are creation and annihilation quasiparticle operators, i is a single-particle state in a spherical mean field,ī is a timeconjugated state.Direct application of QRPA is not justified in the region where the transition takes place from spherical nuclei to deformed ones that is revealed in lowering the energies of the first 2 + -states (e.g., from 1.2 MeV in Sn isotopes up to 0.32 MeV in 120 Xe) and at the same time in increasing B(E2, 2). Applying the standard QRPA yields the values Σ ϕ 2 smaller then but comparable with Σ ψ 2 that necessitates to modify QRPA conformably.Several modification of RPA, included the particlehole RPA and QRPA, have been suggested which take into account GSC more consistently [2][3][4][5][6][7][8]. The main idea of our modification of QRPA (MQRPA) was formulated many years ago [9,10] and was developed further in [11,12]. We construct special equations like RPA for amplitudes ψ and ϕ of the collective quadrupole phonon D μ , Eq. (1), which give very small values of Σ ϕ 2 , i.e. with small GSC in the fermion space. However, after mapping the D-phonons and PV onto the boson space the boson Hamiltonian proves to be such that its diagonalization a e-mail: efimov98@mail.ru leads to a rather complicated ground state function comprising apart from the boson vacuum (BV) two, three and more quadrupole bosons. Thus, if one returned from the boson space to the fermion one the ground state in this space would turn out to be strongly correlated.Transition to the boson description is implemented following the Interacting Boson Model (IBM) in its first variant (IBM1 or SU (6) wherêIn Eqs. (2) Article available at

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Do we understand IBM parameters?

Cited by 40 publications

References 38 publications

Microscopic calculation of the parameters of the interacting Bose-Fermi Approximation for nondegenerate orbits

Microscopic calculation of the parameters of the interacting Bose-Fermi Approximation for nondegenerate orbits

Microscopic description of absolute values for B(E2) within IBM

Collective states of even Xe isotopes in IBM+MQRPA

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